Details on Acronym: HLS | |
| HLS | (Herschel Lensing Survey) |
| ***** | Avoid the usage of HLS, prefer [RRE2012] |
| Origin | of the Acronym: A = Assigned by the author(s) |
Details on Acronym: [RRE2012] | |
| [RRE2012] | (Rawle+Rex+Egami+, 2012)= HLS |
| Write: | <<[RRE2012] HLSJHHMMSS+DDMMSS>> |
| N: | 6 (SIMBAD class: Galaxy) |
| Note: | Dust properties of galaxies in two massive clusters at z∼0.3 from the Herschel Lensing Survey (HLS). |
| in source: | NAME Bullet Cluster |
| Ref: | =2012ApJ...756..106R |
| by | RAWLE T.D. , REX M., EGAMI E., CHUNG S.M., PEREZ-GONZALEZ P.G., SMAIL I., WALTH G., ALTIERI B., APPLETON P., BERCIANO ALBA A., BLAIN A.W., DESSAUGES-ZAVADSKY M., FADDA D., GONZALEZ A.H., PEREIRA M.J., VALTCHANOV I., VAN DER WERF P.P., ZEMCOV M. |
| Astrophys. J., 756, 106 (2012) | |
| Discovery of "Warm dust" galaxies in clusters at z ~ 0.3: evidence for stripping of cool dust in the dense environment? | |
| o | Table 3: <[RRE2012] HLSJHHMMSS+DDMMSS> N=6 |
| Origin | of the Acronym: S = Created by Simbad, the CDS Database |